Counts in cells are used to analyse the higher order properties of the statistics of the EDSGC survey. The probability distribution is obtained from an equal area projection source catalog with infinite oversampling over the range 0.015^\circ-2^\circ. The factorial moments of the resulting distribution and the s_N's characterizing the non-Gaussian nature of the distribution are extracted. These results are compared to previous results from the APM survey, and to theoretical results from perturbation theory. The deprojected 3D values corresponding to the s_N's are also determined. We find that the 3D values match the scaling relation for strongly nonlinear clustering found in N-body simulations remarkably well, suggesting that the galaxies a...
The consequences of models of structure formation for higher-order (n-point) galaxy correlation func...
For a given statistic, A, the cosmic distribution function, Upsilon(VA), is the probability of measu...
We present measurements of the higher-order clustering of red and blue galaxies as a function of sca...
We measure moments of the galaxy count probability distribution function in the Two-degree Field Gal...
We measure the skewness (S_3) and kurtosis (S_4) of the Count Probability Distribution Function (CPD...
We measure moments of the galaxy count probability distribution function in the Two-degree Field Gal...
We measure moments of the galaxy count probability distribution function in the two-degree field gal...
We apply a new statistics, the factorial moment correlators, to density maps obtained from the APM s...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
We use the two-degree field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
Fractal properties are usually characterized by means of various statistical tools which deal with s...
We investigate the spatial clustering of galaxies in the PSCz galaxy redshift survey, as revealed by...
We use the 2MASS extended source catalogue to determine angular correlation functions, w_p, to high ...
Higher order statistics are investigated in ($\Omega$)CDM universes by analyzing $500\mpc$ high reso...
The consequences of models of structure formation for higher-order (n-point) galaxy correlation func...
For a given statistic, A, the cosmic distribution function, Upsilon(VA), is the probability of measu...
We present measurements of the higher-order clustering of red and blue galaxies as a function of sca...
We measure moments of the galaxy count probability distribution function in the Two-degree Field Gal...
We measure the skewness (S_3) and kurtosis (S_4) of the Count Probability Distribution Function (CPD...
We measure moments of the galaxy count probability distribution function in the Two-degree Field Gal...
We measure moments of the galaxy count probability distribution function in the two-degree field gal...
We apply a new statistics, the factorial moment correlators, to density maps obtained from the APM s...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
We use the two-degree field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
Fractal properties are usually characterized by means of various statistical tools which deal with s...
We investigate the spatial clustering of galaxies in the PSCz galaxy redshift survey, as revealed by...
We use the 2MASS extended source catalogue to determine angular correlation functions, w_p, to high ...
Higher order statistics are investigated in ($\Omega$)CDM universes by analyzing $500\mpc$ high reso...
The consequences of models of structure formation for higher-order (n-point) galaxy correlation func...
For a given statistic, A, the cosmic distribution function, Upsilon(VA), is the probability of measu...
We present measurements of the higher-order clustering of red and blue galaxies as a function of sca...